Classical Mechanics Flashcards

1
Q

Define the Frictional force.

A

Ff = μFN, where FN is the normal force and μ is the frictional coefficient.

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2
Q

Give the x- and y- equations of motions for a projectile in motion.

A

x(t) = v0xt + x0 and y(t) = -½gt2 + v0yt + y0

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3
Q

Give a formula relating the initial and final velocities of an object, its acceleration and the change in position between the initial and final states, if acceleration is constant.

A

v2f - v2i = 2aΔy.

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4
Q

In terms of circular motion, if its tangential acceleration is zero, then its tangential velocity is constant; it is moving in uniform circular motion about the center of the circle. Give the radial acceleration and the centripetal force.

A

a = v2/r , Fcent. = mv2/r

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5
Q

State the concept of conservation of energy.

A

If an object acted on only conservation forces, the sum of its kinetic and potential energies is constant along the object’s path.

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6
Q

What are conservative forces?

A

A force to which you can associate a (time-independent) potential energy.

The work done by these forces is independent of the path taken between the starting and ending points.

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7
Q

General principle:

If you want to know how fast or how far someting goes, use _____________________.

If you want to know how much time something takes, use _______________.

A

Conservation of Energy.

Kinematics.

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8
Q

Give the formula of translational kinetic energy.

A

T = ½mv2.

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9
Q

Give the formula of rotational kinetic energy.

A

KErotational = ½Iω2.

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10
Q

Give the formula for Gravitational potential energy on Earth.

A

Ugrav. = mgh

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11
Q

Give the formula of the potential energy of a spring.

A

Uspring = ½kx2.

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12
Q

For any conservative force F, the change in potential energy ΔU between a and b is

A

ΔU = - ∫ F·dl, where the integral goes from a to b.

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13
Q

Give the gravitational force between two masses m1 and m2.

A

Fgrav = Gm1m2/r2 r^.

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14
Q

Give a alternate formula of ΔU = - ∫ F·dl.

A

F = -U.

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15
Q

If the object rolls without slipping, then its linear velocity and angular velocity are related how?

A

v = Rω.

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16
Q

Give a formula of work, due to non conservative forces, and energy.

A

Ei + Wnon conservative = Ef.

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17
Q

Give the work energy theorem.

A

Wconservative = ΔKE

18
Q

Give the general defintion of work.

A

W = ∫ F·dl.

19
Q

What can be applied if Fext = 0 in a system?

A

Fext = , by Newton’s second law.

Momentum is conserved.

20
Q

If things are colliding, try ____________________________ first.

A

Conservation of Momentum.

21
Q

The angular momentum of a point particle of linear momentum is defined by

A

L = r x p.

22
Q

The angular momentum of a extended body of linear momentum is defined by

A

L = Iw.

23
Q

The analogue of the force F for rotational motion is

A

Torque.

τ = r x F

24
Q

The analogues of the equations p = mv and F = dp/dt, in scalar forms are

A

L = Iw and τ = dL/dt.

25
Q

The angular momentum vector L is generally parallel to the ________________, which points along the axis of rotation, just like an object’s linear momentum is parallel to its velocity.

A

angular velocity w

26
Q

Is a reference frame rotating at constant angular velocity inertial or not?

A

Not, but one can still write a formula resembling Newton’s second law at the price of introducing “fictitious” forces.

27
Q

In a rotating frame, this force is responsible for the deviaiton of true g in a non inertial reference frame.

A

The centrifugal force.

Fcentrifugal = -mΩ2r.

28
Q

In a rotating frame, this force is responsible for the curvature trajectory of bullets and hurricanes.

A

The Coriolis force.

FCoriolis = -2mΩ x v.

29
Q

Define the moment of inertia of a point particle of mass m.

A

I = mr2.

30
Q

Define the moment of interia of a rigid body.

A

I = ∫ r2 dm.

31
Q

Conceptually, objects with more mass further from the axis of rotation are _______ to rotate and have a _____ moment of interia.

A

“harder”, larger.

32
Q

Define the parallel axis theorem which is used for moments of interia.

A

I = Icm + Mr2.

33
Q

Define the center of mass of an extended object of mass M.

A

rCM = ∫ r dm / M

34
Q

Define the center of mass formula for point particles.

A

rCM = Σi rimi / M

35
Q

Define the general Lagrangian formula of a system.

A

L(q,q̇,t) = T - U.

36
Q

Define the general Euler - Lagrange equations.

A

d/dt (∂L/∂q̇) = ∂L/∂q.

37
Q

Define the momentum conjugate to q.

A

pi ≡ ∂L/∂q̇

38
Q

Iff the Lagrangian is independent of a coordinate q, the corresponding conjugate momentum ∂L/∂q̇ is what?

A

conserved.

d/dt(∂L/∂q̇) = 0

∂L/∂q̇ is constant.

39
Q

If U does not depend explicitly on velocities or time, define the Hamiltonian.

A

H = T + U.

40
Q

Give the general definition of the Hamiltonian.

A

H(p,q) = Σpii - L

41
Q

Give Hamilton’s equations.

A

ṗ = - ∂H/∂q, q̇ = ∂H/∂p

42
Q

Iff the Hamiltonian is independent of a coordinate q, the corresponding conjugate momentum p is what?

A

conserved.

ṗ = 0.